A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light...
A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
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Author / Creator
D'Antonio, S , Palomba, C , Frasca, S , Intini, G , La Rosa, I , Leaci, P , Mastrogiovanni, S , Miller, A , Muciaccia, F , Piccinni, O J and Singhal, A
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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As a consequence of superradiant instability induced in Kerr black holes, ultra-light boson clouds can be a source of persistent gravitational waves, potentially detectable by current and future gravitational-wave detectors. These signals have been predicted to be nearly monochromatic, with a small steady frequency increase (spin-up), but given the...
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Full title
A semi-coherent analysis method to search for continuous gravitational waves emitted by ultra-light boson clouds around spinning black holes
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TN_cdi_proquest_journals_2110115132
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2110115132
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E-ISSN
2331-8422
